The hydrodynamics of dead radio galaxies

By C. Reynolds, S. Heinz, M. Begelman. 2002

151 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/7898d98d4e944b759d82c2d377b8004ba0354bb1

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In Astronomy and Astrophysics

1. L. Hernquist
2. Volker Springel
3. P. Torrey
4. M. Vogelsberger
5. Shy Genel
6. P. Hopkins
7. D. Nelson
8. F. Marinacci

In Nuclear and High Energy Physics

1. A. C. Fabian
2. L. Hernquist
3. Volker Springel
4. M. Vogelsberger
5. T. Di Matteo
6. P. Torrey
7. Shy Genel
8. D. Nelson

Citations in the corpus

• Simulating galaxy formation with black hole driven thermal and kinetic feedback (2016, background): “…many different approaches for ‘radio mode’ activity have been taken, often using bipolar outflows in idealized simulations of hydrostatic haloes (Reynolds et al. 2002; Basson & Alexander 2003; Omma et al. 2004; Ruszkowski et al. 2004; Zanni et al. 2005; Brighenti & Mathews 2006; Brüggen et…”
• The relationship between the optical Hα filaments and the X‐ray emission in the core of the Perseus cluster (2003, background): “Numerical simulations of the intracluster medium will needto ensure that the gas has an effective viscosity at this level (th simulations of e.g. Reynolds et al 2002 show turbulence) and to confirm that the flow is indeed laminar.”
• Heating cooling flows with jets (2003, methodology): “Several sets of simulations of AGN/cooling-flow interaction have appeared in the literature (Churazov et al. 2001; Quilis et al. 2001; Brüggen & Kaiser 2001, 2002; Reynolds et al. 2001, 2002; Brüggen et al. 2002; Basson & Alexander 2003).”
• Heating Hot Atmospheres with Active Galactic Nuclei (2007, background): “Simulations show that buoyant cavities can heat the surrounding gas as they rise through a cluster atmosphere (Brüggen & Kaiser 2002; Reynolds et al. 2002).”
• Accretion onto the Supermassive Black Hole in M87 (2002, methodology): “We take r2 to be the crosssectional area of the bubble inflated by the jet around the center (which, for simplicity, we take to be spherical; see Churazov et al. 2001; Reynolds et al. 2002).”
• AGN Feedback and Cooling Flows: Problems with Simple Hydrodynamic Models (2005, methodology): “…have explored the buoyant evolution of the cocoon after its supersonic expansion phase (Churazov et al. 2001; Brüggen & Kaiser 2001, 2002; Reynolds et al. 2002; Basson & Alexander 2003; Omma et al. 2004; Omma & Binney 2004; Dalla Vecchia et al. 2004; Robinson et al. 2004; Zanni et al.…”
• Outflows in Active Galactic Nucleus/Starburst-Composite Ultraluminous Infrared Galaxies (2005, background): “Outflows from AGNs have recently been invoked as global heat (or entropy) sources for the intracluster medium (ICM) at both small and large radii (e.g., Reynolds et al. 2002; Roychowdhury et al. 2004 and references therein).”